A) To take pictures of the moon. B) To magnify objects directly. C) To track satellites. D) To gather and focus light.
A) The length of the telescope tube. B) The diameter of the objective lens or mirror. C) The weight of the telescope. D) The magnification power of the eyepiece.
A) Reflecting telescope. B) Refracting telescope. C) Catadioptric telescope. D) Radio telescope.
A) Refracting telescope. B) Catadioptric telescope. C) Radio telescope. D) Reflecting telescope.
A) The distance between the lens/mirror and the focal point. B) The length of the telescope tube. C) The width of the lens/mirror. D) The magnification of the telescope.
A) To magnify the image formed by the objective. B) To filter out unwanted light. C) To gather light from distant objects. D) To focus light into the telescope.
A) Focal length of objective + Focal length of eyepiece. B) Focal length of objective / Focal length of eyepiece. C) Focal length of objective * Focal length of eyepiece. D) Focal length of eyepiece / Focal length of objective.
A) The clarity of the telescope lens. B) The steadiness of the atmosphere. C) The observer's eyesight. D) The brightness of the target object.
A) The natural light emitted by stars. B) The reflection of sunlight off the moon. C) Excessive artificial light that obscures the night sky. D) The aurora borealis.
A) Equatorial mount. B) Eyepiece mount. C) Mirror mount. D) Lens mount.
A) Allows the telescope to rotate horizontally only. B) Allows the telescope to move up and down only. C) Keeps the telescope perfectly still. D) Tracks celestial objects as the Earth rotates.
A) Double stars. B) The Moon's craters. C) Nebula. D) Planets.
A) Star clusters. B) Planets. C) Galaxies. D) Nebula.
A) Calculating the telescope's magnification. B) Aligning the optical elements of a telescope. C) Polishing the telescope lens. D) Attaching the telescope to the mount.
A) To increase the telescope's magnification. B) To protect the telescope from dust. C) To make the telescope easier to carry. D) To achieve the sharpest possible image.
A) Automatically tracks stars. B) Magnifies the image more than the eyepiece. C) Helps you locate objects in the sky. D) Filters out light pollution.
A) Solar filter. B) Moon filter. C) Color filter. D) Light pollution filter.
A) Look directly at the Sun. B) Look at a planet. C) Look at the Moon. D) Look at a bright star.
A) To make the telescope more stable. B) To block out light pollution. C) To prevent dew from forming on the lens. D) To protect the telescope from rain.
A) During the day. B) During twilight. C) After the sky is completely dark. D) As soon as the sun sets.
A) Observing stars with a binocular. B) Observing shooting stars. C) Using a star chart to find faint objects. D) Traveling between different star systems.
A) Astronomical Units (AU). B) Light-years. C) Parsecs. D) Millimeters or Inches.
A) Plossl eyepiece. B) Orthoscopic eyepiece. C) Wide-field eyepiece. D) Huygenian eyepiece.
A) Schmidt-Cassegrain telescope. B) Newtonian telescope. C) Maksutov-Cassegrain telescope. D) Dobsonian telescope.
A) Use your breath and a clean shirt. B) Use a specialized lens cleaning solution and cloth. C) Use a paper towel. D) Use regular household cleaner.
A) The faintest star visible through the telescope. B) The distance the telescope can see. C) The brightest star visible through the telescope. D) The maximum magnification of the telescope.
A) Solar flares. B) Electromagnetic radiation. C) Atmospheric turbulence. D) Gravitational waves.
A) Measuring the positions of stars. B) Drawing pictures of celestial objects. C) Taking pictures of celestial objects. D) Studying the chemical composition of stars.
A) To prevent the telescope from drifting. B) To accurately align an equatorial mount. C) To measure the speed of stars. D) To find the North Star.
A) Solar filter. B) Light pollution filter. C) Moon filter. D) Hydrogen-alpha filter. |